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Evolution of the grain size distribution in galactic discs
[article]
2020
arXiv
pre-print
Dust is formed out of stellar material and is constantly affected by different mechanisms occurring in the ISM. Dust grains behave differently under these mechanisms depending on their sizes, and therefore the dust grain size distribution also evolves as part of the dust evolution itself. Following how the grain size distribution evolves is a difficult computing task that is just recently being overtaking. Smoothed particle hydrodynamic (SPH) simulations of a single galaxy as well as
arXiv:2002.01945v1
fatcat:crh2d7eejbbmhpjhaz4jxti67e